Computes black hole images in Hernquist DM halos across thin-disk and spherical accretion models, finding enlarged critical curves and model-dependent brightness suppression usable for DM constraints.
Synge, Monthly Notices of the Royal Astronomical Society131, 463 (1966)
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Probing Hernquist dark matter through the optical appearance of black holes: A comprehensive study of various accretions
Computes black hole images in Hernquist DM halos across thin-disk and spherical accretion models, finding enlarged critical curves and model-dependent brightness suppression usable for DM constraints.